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dc.contributor.authorWOLF, Sebastian
hal.structure.identifierInstitut de Planétologie et d'Astrophysique de Grenoble [IPAG ]
dc.contributor.authorMALBET, Fabien
dc.contributor.authorALEXANDER, Richard
hal.structure.identifierInstitut de Planétologie et d'Astrophysique de Grenoble [IPAG ]
dc.contributor.authorBERGER, Jean-Philippe
dc.contributor.authorCREECH-EAKMAN, Michelle
hal.structure.identifierInstitut de Planétologie et d'Astrophysique de Grenoble [IPAG ]
dc.contributor.authorDUCHENE, Gaspard
hal.structure.identifierAMOR 2012
dc.contributor.authorDUTREY, Anne
dc.contributor.authorMORDASINI, Christophe
hal.structure.identifierAstrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)]
dc.contributor.authorPANTIN, Eric
hal.structure.identifierUniversity of Exeter
dc.contributor.authorPONT, Frederic
dc.contributor.authorPOTT, Joerg-Uwe
hal.structure.identifierINAF - Osservatorio Astrofisico di Arcetri [OAA]
dc.contributor.authorTATULLI, Eric
hal.structure.identifierINAF - Osservatorio Astrofisico di Arcetri [OAA]
dc.contributor.authorTESTI, Leonardo
dc.date.created2012-03-28
dc.date.issued2012
dc.identifier.issn0935-4956
dc.description.abstractEnWe present a review of the interplay between the evolution of circumstellar disks and the formation of planets, both from the perspective of theoretical models and dedicated observations. Based on this, we identify and discuss fundamental questions concerning the formation and evolution of circumstellar disks and planets which can be addressed in the near future with optical and infrared long-baseline interferometers. Furthermore, the importance of complementary observations with long-baseline (sub)millimeter interferometers and high-sensitivity infrared observatories is outlined.
dc.language.isoen
dc.publisherSpringer Verlag
dc.subject.enInstrumentation and Methods for Astrophysics
dc.subject.enEarth and Planetary Astrophysics
dc.subject.enAstrophysics
dc.subject.enSolar and Stellar Astrophysics
dc.title.enCircumstellar disks and planets. Science cases for next-generation optical/infrared long-baseline interferometers
dc.typeArticle de revue
dc.identifier.doi10.1007/s00159-012-0052-1
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]/Instrumentation et méthodes pour l'astrophysique [astro-ph.IM]
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Instrumentation et méthodes pour l'astrophysique [astro-ph.IM]
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]/Planétologie et astrophysique de la terre [astro-ph.EP]
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Planétologie et astrophysique de la terre [astro-ph.EP]
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]/Astrophysique stellaire et solaire [astro-ph.SR]
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Astrophysique stellaire et solaire [astro-ph.SR]
dc.identifier.arxiv1203.6271
bordeaux.journalAstronomy and Astrophysics Review
bordeaux.page52
bordeaux.volume20
bordeaux.peerReviewedoui
hal.identifierhal-00685526
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-00685526v1
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